In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 37, no. 2
D. Pecinová - P. Pecina
Detaily:
Rok, strany: 2007, 83 - 106
O článku:
The theoretical construction of a model of the range distribution of
computation of five important parameters connected with the structure
of meteor showers as well as physical features of meteoroids related
to them. These are: the mass distribution index, s, the shower flux
density, Θm0, the ionization coefficient,
β, the Levin's
parameter (self-similarity parameter), µ, the product of the
shape-density coefficient, K, and the ablation parameter, σ.
We present details of the numerical model in the article which proved
to be a good explanation for the real observed process. The model (RaDiM)
is based on the overdense echoes of shower meteors. It makes use of the
long-term series of data that have been collected by the Ondřejov
meteor radar during almost five decades. Its application and relevant
results will be described in subsequent articles.
Ako citovať:
ISO 690:
Pecinová, D., Pecina, P. 2007. Radar meteors range distribution model. I. Theory. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 37, no.2, pp. 83-106. 1335-1842.
APA:
Pecinová, D., Pecina, P. (2007). Radar meteors range distribution model. I. Theory. Contributions of the Astronomical Observatory Skalnaté Pleso, 37(2), 83-106. 1335-1842.